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arXiv · 1210.0001

Noether symmetry of F(T) cosmology with quintessence and phantom scalar fields

Mubasher Jamil·D. Momeni·R. Myrzakulov
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Abstract

In this paper, we investigate the Noether symmetries of $F(T)$ cosmology involving matter and dark energy. In this model, the dark energy is represented by a canonical scalar field with a potential. Two special cases for dark energy are considered including phantom energy and quintessence. We obtain $F(T)\sim T^{3/4},$ and the scalar potential $V(ϕ)\simϕ^2$ for both models of dark energy and discuss quantum picture of this model. Some astrophysical implications are also discussed.

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Mubasher Jamil, D. Momeni, R. Myrzakulov. 2012-09-28. Noether symmetry of F(T) cosmology with quintessence and phantom scalar fields. https://doi.org/10.1140/epjc%2Fs10052-012-2137-4

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